Zobrazeno 1 - 10
of 1 609
pro vyhledávání: '"E Rubinstein"'
Autor:
David A. Neufeld, P. Manoj, Himanshu Tyagi, Mayank Narang, Dan M. Watson, S. Thomas Megeath, Ewine F. Van Dishoeck, Robert A. Gutermuth, Thomas Stanke, Yao-Lun Yang, Adam E. Rubinstein, Guillem Anglada, Henrik Beuther, Alessio Caratti o Garatti, Neal J. Evans II, Samuel Federman, William J. Fischer, Joel Green, Pamela Klaassen, Leslie W. Looney, Mayra Osorio, Pooneh Nazari, John J. Tobin, Łukasz Tychoniec, Scott Wolk
Publikováno v:
The Astrophysical Journal Letters, Vol 966, Iss 2, p L22 (2024)
Using the MIRI medium-resolution spectrometer on JWST, we have detected pure rotational, suprathermal OH emissions from the vicinity of the intermediate-mass protostar HOPS 370 (OMC2/FIR3). These emissions are observed from shocked knots in a jet/out
Externí odkaz:
https://doaj.org/article/37e0b6f0cf5b4c4cb675aeefe7773f5c
Autor:
Mayank Narang, P. Manoj, Himanshu Tyagi, Dan M. Watson, S. Thomas Megeath, Samuel Federman, Adam E. Rubinstein, Robert Gutermuth, Alessio Caratti o Garatti, Henrik Beuther, Tyler L. Bourke, Ewine F. Van Dishoeck, Neal J. Evans II, Guillem Anglada, Mayra Osorio, Thomas Stanke, James Muzerolle, Leslie W. Looney, Yao-Lun Yang, Pamela Klaassen, Nicole Karnath, Prabhani Atnagulov, Nashanty Brunken, William J. Fischer, Elise Furlan, Joel Green, Nolan Habel, Lee Hartmann, Hendrik Linz, Pooneh Nazari, Riwaj Pokhrel, Rohan Rahatgaonkar, Will R. M. Rocha, Patrick Sheehan, Katerina Slavicinska, Amelia M. Stutz, John J. Tobin, Lukasz Tychoniec, Scott Wolk
Publikováno v:
The Astrophysical Journal Letters, Vol 962, Iss 1, p L16 (2024)
Investigating Protostellar Accretion (IPA) is a JWST Cycle 1 GO program that uses NIRSpec integral field units and MIRI Medium Resolution Spectrograph to obtain 2.9–28 μ m spectral cubes of young, deeply embedded protostars with luminosities of 0.
Externí odkaz:
https://doaj.org/article/dfdbf40e59a34686b7118e4faaf594a3
Autor:
Adam E. Rubinstein, Neal J. Evans II, Himanshu Tyagi, Mayank Narang, Pooneh Nazari, Robert Gutermuth, Samuel Federman, P. Manoj, Joel D. Green, Dan M. Watson, S. Thomas Megeath, Will R. M. Rocha, Nashanty G. C. Brunken, Katerina Slavicinska, Ewine F. van Dishoeck, Henrik Beuther, Tyler L. Bourke, Alessio Caratti o Garatti, Lee Hartmann, Pamela Klaassen, Hendrik Linz, Leslie W. Looney, James Muzerolle, Thomas Stanke, John J. Tobin, Scott J. Wolk, Yao-Lun Yang
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 112 (2024)
We investigate the bright CO fundamental emission in the central regions of five protostars in their primary mass assembly phase using new observations from JWST’s Near-Infrared Spectrograph and Mid-Infrared Instrument. CO line emission images and
Externí odkaz:
https://doaj.org/article/88875499e1f440799610eb981466f866
Autor:
Nicole Karnath, Adam E. Rubinstein, Samuel Federman, Alice C. Quillen, Joel D. Green, Edward T. Chambers, Dan M. Watson, S. Thomas Megeath, Simon Coudé, Matthias Justen, Mayank Narang, Steve Goldman, John J. Tobin
Publikováno v:
The Astrophysical Journal, Vol 974, Iss 1, p 65 (2024)
We present a combined Stratospheric Observatory for Infrared Astronomy (SOFIA) and two-epoch Hubble Space Telescope (HST) study of the region NGC 2071 IR containing the outflow from the protostar HOPS 361-A (NGC 2071 IRS 1). New [O i ] 63 μ m spectr
Externí odkaz:
https://doaj.org/article/8e17341c351f4925923ce916034863f9
Autor:
Samuel A. Federman, S. Thomas Megeath, Adam E. Rubinstein, Robert Gutermuth, Mayank Narang, Himanshu Tyagi, P. Manoj, Guillem Anglada, Prabhani Atnagulov, Henrik Beuther, Tyler L. Bourke, Nashanty Brunken, Alessio Caratti o Garatti, Neal J. Evans II, William J. Fischer, Elise Furlan, Joel D. Green, Nolan Habel, Lee Hartmann, Nicole Karnath, Pamela Klaassen, Hendrik Linz, Leslie W. Looney, Mayra Osorio, James Muzerolle Page, Pooneh Nazari, Riwaj Pokhrel, Rohan Rahatgaonkar, Will R. M. Rocha, Patrick Sheehan, Katerina Slavicinska, Thomas Stanke, Amelia M. Stutz, John J. Tobin, Lukasz Tychoniec, Ewine F. Van Dishoeck, Dan M. Watson, Scott Wolk, Yao-Lun Yang
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 41 (2024)
Investigating Protostellar Accretion is a Cycle 1 JWST program using the NIRSpec+MIRI integral field units to obtain 2.9–28 μ m spectral cubes of five young protostars with luminosities of 0.2–10,000 L _⊙ in their primary accretion phase. This
Externí odkaz:
https://doaj.org/article/e06290ca3a554a0981e03c352197ef13
Autor:
Adam E. Rubinstein, Nicole Karnath, Alice C. Quillen, Samuel Federman, Joel D. Green, Edward T. Chambers, Dan M. Watson, S. Thomas Megeath
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 1, p 39 (2023)
We present a two-epoch Hubble Space Telescope study of NGC 2071 IR highlighting HOPS 361-C, a protostar producing an arced 0.2 parsec-scale jet. The proper motions for the brightest knots decrease from 350 to 100 km s ^−1 with increasing distance f
Externí odkaz:
https://doaj.org/article/c17017a334b24d78b1b73b5fed360aee
Publikováno v:
Bulletin of the Moscow State Regional University (Economics). :15-22
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6b7d8f39e5788fa142ea33293d0c8896
https://doi.org/10.18384/2310-6646-2022-1-15-22
https://doi.org/10.18384/2310-6646-2022-1-15-22
Autor:
Ashley E Rubinstein, Skylar Gay, Christine B Peterson, Charles V Kingsley, Ramesh C Tailor, Julianne M Pollard-Larkin, Adam D Melancon, David S Followill, Laurence E Court
Publikováno v:
PLoS ONE, Vol 13, Iss 11, p e0205803 (2018)
Strong magnetic fields affect radiation dose deposition in MRI-guided radiation therapy systems, particularly at interfaces between tissues of differing densities such as those in the thorax. In this study, we evaluated the impact of a 1.5 T magnetic
Externí odkaz:
https://doaj.org/article/5306a58139fc4822b64cb85c6253d066
Autor:
Adam E. Rubinstein, Nicole Karnath, Alice C. Quillen, Samuel Federman, Joel D. Green, Edward T. Chambers, Dan M. Watson, S. Thomas Megeath
We present a two-epoch Hubble Space Telescope (HST) study of NGC 2071 IR highlighting HOPS 361-C, a protostar producing an arced 0.2 parsec-scale jet. Proper motions for the brightest knots decrease from 350 to 100 km/s with increasing distance from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b97937c96da4879ac979b125aa2635e0
http://arxiv.org/abs/2211.12599
http://arxiv.org/abs/2211.12599
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